Recalibration of Luminosity-HI Linewidth Relations and H_0

dc.creatorTully, R. Brent
dc.date1998-02-03
dc.date.accessioned2026-07-07T02:25:57Z
dc.date.available2026-07-07T02:25:57Z
dc.descriptionA recalibration of the luminosity-linewidth technique is discussed which introduces (i) new cluster calibration data, (ii) new corrections for reddening as a function of inclination, and (iii) a new zero-point calibration using 13 galaxies with distances determined via the cepheid period-luminosity method. It is found that H_0= 82 +/- 16 km/s/Mpc (95% confidence)
dc.description7 pages with 3 figures encapsulated in the .ps file
dc.identifierhttps://arxiv.org/abs/astro-ph/9802027
dc.identifierhttp://arxiv.org/abs/astro-ph/9802027
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12084
dc.subjectAstrophysics
dc.titleRecalibration of Luminosity-HI Linewidth Relations and H_0
dc.typetext

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